Calibration of the ISOCAM LW2 and LW3 filters using ELAIS stars

Details Calibration of the ISOCAM LW2 and LW3 filters using ELAIS stars Calibration of the ISOCAM LW2 and LW3 filters using ELAIS stars

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999esasp.427...85m&link_type=abstract

The Universe as Seen by ISO. Eds. P. Cox & M. F. Kessler. ESA-SP 427., p. 85

Computer Science

1

Isocam, Stellar Magnitudes

Scientific paper

By using bolometric magnitudes and a blackbody approximation we estimate expected fluxes at 6.7μm and 15μm for SIMBAD and Hipparcos stars located in the ELAIS fields. Our model is tested against IRAS 12μm observations and shown to work well. By comparing the expected fluxes with ISO instrumental units we obtain sensitivity factors of 1.78mJy/(ADU/g/s) and 1.42mJy/(ADU/g/s) at 6.7μm and 15μm respectively. Colour correction factors are also obtained.

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